Coexistence of early-time inflation and late-time acceleration with scalar fields in theory of F(G,T) gravity

DOI10.1142/S0218271818500785zbMath1430.83073OpenAlexW2789146745MaRDI QIDQ5216116

A. I. Keskin

Publication date: 14 February 2020

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271818500785

zbMATH Keywords

inflationdark energy\(F(G, T)\) gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Dark matter and dark energy (83C56)

Related Items (3)

Cosmic acceleration with tachyon field ⋮ The inflationary era of the universe via Tsallis cosmology ⋮ Self-gravitating gaseous spheres in 5D framework

Cites Work

• Universal thermodynamics in different gravity theories: Conditions for generalized second law of thermodynamics and thermodynamical equilibrium on the horizons
• Generalized second law of thermodynamics in \(f(T)\) gravity with entropy corrections
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• \(f(R)\) theories
• Universal thermodynamics in different gravity theories: modified entropy on the horizons
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Thermodynamics of apparent horizon in brane world scenario
• Extended scalar–tensor theory and thermodynamics in teleparallel framework
• The generalized second law of thermodynamics for interacting f(R) gravity
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• A unified picture of cosmological entropy on apparent horizon in F(R, G) gravity
• Hawking radiation of an apparent horizon in a FRW universe
• Thermodynamics of Spacetime: The Einstein Equation of State
• Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes
• Dark energy problem: from phantom theory to modified Gauss–Bonnet gravity

This page was built for publication: Coexistence of early-time inflation and late-time acceleration with scalar fields in theory of F(G,T) gravity